Brian Topper,1,2 Alexander Neumann,2 Alexander R. Albrechthttps://orcid.org/0000-0001-7641-9332,1 Angel S. Flores,3 Stefan Kuhn,4 Denny Häßner,4 Sigrun Hein,4 Christian Hupel,4 Johannes Nold,4 Nicoletta Haarlammert,4 Thomas Schreiber,4 Mansoor Sheik-Bahaehttps://orcid.org/0000-0001-5703-3653,1 Arash Mafi1,5
1Univ. of New Mexico (United States) 2Ctr. for High Technology Materials, Univ. of New Mexico (United States) 3Air Force Research Lab. (United States) 4Fraunhofer-Institut für Angewandte Optik und Feinmechanik IOF (Germany) 5 Ctr. for High Technology Materials, Univ. of New Mexico (United States)
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Recent years have seen silica emerge as a viable material for optical refrigeration with potential applications in directed energy, integrated photonics, and precision metrology. Proper characterization of potential composition profiles is vital for optimization. Here, static photoluminescence spectroscopy of a Yb, Al co-doped silica sample over the temperature range 80 K to 300 K reveals the emission lineshape is dependent on the excitation wavelength. The impact this has on extracted laser cooling parameters is discussed.
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Brian Topper, Alexander Neumann, Alexander R. Albrecht, Angel S. Flores, Stefan Kuhn, Denny Häßner, Sigrun Hein, Christian Hupel, Johannes Nold, Nicoletta Haarlammert, Thomas Schreiber, Mansoor Sheik-Bahae, Arash Mafi, "Laser cooling silica: current status and future prospects," Proc. SPIE 12437, Photonic Heat Engines: Science and Applications V, 1243703 (15 March 2023); https://doi.org/10.1117/12.2655228